Effect of width, amplitude, and position of a core mantle boundary hot spot on core convection and dynamo action

Dietrich, W, Wicht, J and Hori, K (2015) Effect of width, amplitude, and position of a core mantle boundary hot spot on core convection and dynamo action. Progress in Earth and Planetary Science, 2. 35. ISSN 2197-4284

Abstract

Metadata

Authors/Creators:
  • Dietrich, W
  • Wicht, J
  • Hori, K
Copyright, Publisher and Additional Information: © 2015 Dietrich et al. Open Access. This article is distributed under the terms of the Creative Commons Attribution 4.0 International License (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted use, distribution, and reproduction in any medium, provided you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons license, and indicate if changes were made.
Keywords: Core Convection; Geodynamo; Ancient Martian dynamo; Inhomogeneous CMB heat flux; Numerical simulation
Dates:
  • Published: 4 November 2015
  • Accepted: 14 October 2015
Institution: The University of Leeds
Academic Units: The University of Leeds > Faculty of Maths and Physical Sciences (Leeds) > School of Mathematics (Leeds) > Applied Mathematics (Leeds)
Depositing User: Symplectic Publications
Date Deposited: 05 Nov 2015 11:34
Last Modified: 12 Feb 2019 13:45
Published Version: http://dx.doi.org/10.1186/s40645-015-0065-2
Status: Published
Publisher: Springer Verlag
Identification Number: https://doi.org/10.1186/s40645-015-0065-2

Share / Export

Statistics